[987] | 1 | \chapter{Physical parameterizations of the generic model: some references} |
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| 2 | |
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| 3 | \label{sc:phystd} |
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| 4 | |
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| 5 | \section{General} |
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| 6 | |
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| 7 | The Generic Climate Model uses a large number of physical parameterizations based on various scientific theories. Some also use specific numerical methods. A list of these parameterizations is given below, along with the most appropriate references for each one. Most of these documents can be found at\\ |
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| 8 | \verb+http://www.lmd.jussieu.fr/mars.html+. |
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| 9 | |
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| 10 | \paragraph{General references:} |
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| 11 | No documents attempt to give a complete scientific description of the current |
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| 12 | version of the GCM. Here's a reference to a Mars GCM description: |
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| 13 | \begin{itemize} |
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| 14 | \item {\it Forget et al.} [1999] (article |
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| 15 | published in the JGR) |
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| 16 | \item ``Updated Detailed Design Document for the Model'' |
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| 17 | (ESA contract, Work Package 6, 1999, available on the web) |
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| 18 | which is simply a compilation of the preceding article with |
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| 19 | a few additions that were published separately. |
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| 20 | \end{itemize} |
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| 21 | |
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| 22 | \nocite{Forg:99} |
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| 23 | |
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| 24 | \section{Radiative transfer} |
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| 25 | |
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| 26 | The radiative transfer parameterizations are used to calculate the heating |
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| 27 | and cooling ratios in the atmosphere and the radiative flux at the surface. |
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| 28 | |
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| 29 | [TO WRITE: IMPORTANT SECTION - REFERENCES HERE ARE FOR MARS ONLY] |
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| 30 | |
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| 31 | %\end{itemize} |
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| 32 | |
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| 33 | |
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| 34 | \subsection{\bf Absorption/emission and diffusion by dust:} |
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| 35 | |
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| 36 | \subsubsection*{Dust spatial distribution} |
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| 37 | (\verb+ dustopacity+) |
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| 38 | |
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| 39 | \begin{itemize} |
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| 40 | \item Vertical distribution and description of ``MGS'' and ``Viking'' scenarios |
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| 41 | in the ESA report {\it Mars Climate Database V3.0 Detailed Design Document} |
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| 42 | by Lewis et al. (2001), available on the web. |
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| 43 | \item For the ``MY24'' scenario, dust distribution obtained from assimilation |
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| 44 | of TES data is used (and read via the \verb+readtesassim+ routine). |
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| 45 | \end{itemize} |
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| 46 | \nocite{Forg:99,Lewi:99} |
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| 47 | |
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| 48 | \subsubsection*{Thermal IR radiation} |
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| 49 | (\verb+ lwmain+) |
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| 50 | \begin{itemize} |
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| 51 | \item Numerical method: {\it Toon et al.} [1989] |
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| 52 | \item Optical properties of dust: {\it Forget} [1998] |
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| 53 | \nocite{Toon:89,Forg:98grl} |
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| 54 | \end{itemize} |
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| 55 | |
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| 56 | \subsubsection*{Solar radiation} |
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| 57 | (\verb+ swmain+) |
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| 58 | \begin{itemize} |
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| 59 | \item Numerical method: {\it Fouquart and Bonel} [1980] |
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| 60 | \nocite{Fouq:80} |
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| 61 | |
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| 62 | \item Optical properties of dust: |
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| 63 | see the discussion in {\it Forget et al. } [1999], which quotes |
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| 64 | {\it Ockert-Bell et al.} [1997] and {\it Clancy and Lee} [1991]. |
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| 65 | \nocite{Ocke:97,Clan:91} |
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| 66 | \end{itemize} |
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| 67 | |
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| 68 | \section{Subgrid atmospheric dynamical processes} |
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| 69 | |
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| 70 | \subsection{Turbulent diffusion in the upper layer} |
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| 71 | (\verb+ vdifc+) |
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| 72 | |
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| 73 | \begin{itemize} |
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| 74 | \item Implicit numerical scheme in the vertical: |
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| 75 | see the thesis of Laurent Li (LMD, Universit\'e Paris 7, 1990), Appendix C2. |
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| 76 | |
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| 77 | \item Calculation of the turbulent diffusion coefficients: |
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| 78 | {\it Forget et al. } [1999]. |
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| 79 | \end{itemize} |
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| 80 | |
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| 81 | \subsection{Convection} |
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| 82 | (\verb+ convadj+) |
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| 83 | |
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| 84 | See {\it Hourdin et al.} [1993] |
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| 85 | \nocite{Hour:93} |
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| 86 | |
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| 87 | \section{Surface thermal conduction} |
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| 88 | (\verb+soil+) |
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| 89 | |
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| 90 | Thesis of Fr\'ed\'eric Hourdin (LMD, Universit\'e Paris 7, 1992) : |
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| 91 | section 3.3 (equations) and Appendix A (Numerical scheme). |
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| 92 | |
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| 93 | \section{CO$_2$ Condensation} |
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| 94 | |
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| 95 | In {\it Forget et al.} [1998] (article published in Icarus): \\ |
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| 96 | - Numerical method for calculating the condensation and sublimation levels |
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| 97 | at the surface and in the atmosphere (\verb+ newcondens+) |
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| 98 | explained in the appendix. |
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| 99 | \\ |
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| 100 | - Description of the numerical scheme for calculating the evolution of CO$_2$ |
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| 101 | snow emissivity (\verb+co2snow+) explained in section 4.1 |
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| 102 | \nocite{Forg:98} |
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| 103 | |
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| 104 | \section{Tracer transport and sources} |
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| 105 | \begin{itemize} |
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| 106 | \item ``Van-Leer'' transport scheme used in the dynamical part |
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| 107 | (\verb+ tracvl+ and \verb+ vlsplt+ in the dynamical part): |
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| 108 | {\it Hourdin and Armengaud} [1999] \nocite{Hour:99} |
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| 109 | |
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| 110 | \item Transport by turbulent diffusion (in \verb+ vdifc+), convection |
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| 111 | (in \verb+ convadj+), sedimentation (\verb+ sedim+), |
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| 112 | dust lifting by winds (\verb+ dustlift+) : |
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| 113 | see note ``Preliminary design of dust lifting and transport in the Model'' |
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| 114 | (ESA contract, Work Package 4, 1998, available on the web). |
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| 115 | |
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| 116 | |
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| 117 | %\item Simplified water cycle (source in {\tt vdifc}, {\tt |
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| 118 | %watercloud}) : and also see the Maitrise study by Delphine Nobileau, LMD, 2000. |
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| 119 | \item {\bf Watercycle}, see {\it Montmessin et al.} [2004] |
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| 120 | \nocite{Mont:04jgr} |
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| 121 | |
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| 122 | \end{itemize} |
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| 123 | |
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| 124 | |
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